Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission
Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery, the mysteries surrounding their origins remain. Here, we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b, TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, an...
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| creator | Schulte, Jack Rodriguez, Joseph E Bieryla, Allyson Quinn, Samuel N Collins, Karen A Yee, Samuel W Nine, Andrew C Soares-Furtado, Melinda Latham, David W Eastman, Jason D Barkaoui, Khalid Ciardi, David R Dragomir, Diana Everett, Mark E Giacalone, Steven Mireles, Ismael Murgas, Felipe Narita, Norio Shporer, Avi Strakhov, Ivan A Striegel, Stephanie Vaňko, Martin Vowell, Noah Wang, Gavin Ziegler, Carl Bellaver, Michael Benni, Paul Bergeron, Serge Boffin, Henri M. J Briceño, César Clark, Catherine A Collins, Kevin I de Leon, Jerome P Dressing, Courtney D Evans, Phil Esparza-Borges, Emma Fedewa, Jeremy Fukui, Akihiko Gan, Tianjun Gerasimov, Ivan S Hartman, Joel D Gill, Holden Gillon, Michaël Horne, Keith Horta, Ferran Grau Howell, Steve B Isogai, Keisuke Jehin, Emmanuël Jenkins, Jon M Karjalainen, Raine Kielkopf, John F Lester, Kathryn V Littlefield, Colin Lund, Michael B Mann, Andrew W McCormack, Mason Michaels, Edward J Painter, Shane Palle, Enric Parviainen, Hannu Peterson, David-Michael Pozuelos, Francisco J Raup, Zachary Reed, Phillip Relles, Howard M Ricker, George R Savel, Arjun B Schwarz, Richard P Seager, Sara Sefako, Ramotholo Srdoc, Gregor Stockdale, Chris Sullivan, Hannah Timmermans, Mathilde Winn, Joshua N |
| description | Hot Jupiters were many of the first exoplanets discovered in the 1990s, but
in the decades since their discovery, the mysteries surrounding their origins
remain. Here, we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b,
TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and
TOI-5301 b) discovered by NASA's TESS mission and confirmed using ground-based
imaging and spectroscopy. These discoveries are the first in a series of papers
named the Migration and Evolution of giant ExoPlanets (MEEP) survey and are
part of an ongoing effort to build a complete sample of hot Jupiters orbiting
FGK stars, with a limiting Gaia $G$-band magnitude of 12.5. This effort aims to
use homogeneous detection and analysis techniques to generate a set of
precisely measured stellar and planetary properties that is ripe for
statistical analysis. The nine planets presented in this work occupy a range of
masses (0.55 Jupiter masses (M$_{\rm{J}}$) $ |
| doi_str_mv | 10.48550/arxiv.2401.05923 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2401_05923</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2401_05923</sourcerecordid><originalsourceid>FETCH-LOGICAL-a673-eb328870317d76205963b89e0b287a1a28a09a8e0ed63fb4095c6ab30a546d1c3</originalsourceid><addsrcrecordid>eNotj0FPgzAYhnvxYKY_wJPfUQ9goVCKN0OqmxlzybiTj1FmE2iX0s3t32-ipzfv5cnzEPIQ0TARaUpf0J30MYwTGoU0zWN2S4ZS7xx6bQ2gaUEebX-Ynu1gp9F4kCe77tEoP8JTKeX6GRavsNJGwUr99GcorOm0G1QLc-vh87DXXrkROmcH8N8KKrnZQKnH8Uq9Izcd9qO6_98Zqd5lVcyD5dfHonhbBsgzFqiGxUJklEVZm_H4aspZI3JFm1hkGGEskOYoFFUtZ12T0DzdcmwYxTThbbRlM_L4h516673TA7pz_dtdT93sAhByUZ8</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission</title><source>arXiv.org</source><creator>Schulte, Jack ; Rodriguez, Joseph E ; Bieryla, Allyson ; Quinn, Samuel N ; Collins, Karen A ; Yee, Samuel W ; Nine, Andrew C ; Soares-Furtado, Melinda ; Latham, David W ; Eastman, Jason D ; Barkaoui, Khalid ; Ciardi, David R ; Dragomir, Diana ; Everett, Mark E ; Giacalone, Steven ; Mireles, Ismael ; Murgas, Felipe ; Narita, Norio ; Shporer, Avi ; Strakhov, Ivan A ; Striegel, Stephanie ; Vaňko, Martin ; Vowell, Noah ; Wang, Gavin ; Ziegler, Carl ; Bellaver, Michael ; Benni, Paul ; Bergeron, Serge ; Boffin, Henri M. J ; Briceño, César ; Clark, Catherine A ; Collins, Kevin I ; de Leon, Jerome P ; Dressing, Courtney D ; Evans, Phil ; Esparza-Borges, Emma ; Fedewa, Jeremy ; Fukui, Akihiko ; Gan, Tianjun ; Gerasimov, Ivan S ; Hartman, Joel D ; Gill, Holden ; Gillon, Michaël ; Horne, Keith ; Horta, Ferran Grau ; Howell, Steve B ; Isogai, Keisuke ; Jehin, Emmanuël ; Jenkins, Jon M ; Karjalainen, Raine ; Kielkopf, John F ; Lester, Kathryn V ; Littlefield, Colin ; Lund, Michael B ; Mann, Andrew W ; McCormack, Mason ; Michaels, Edward J ; Painter, Shane ; Palle, Enric ; Parviainen, Hannu ; Peterson, David-Michael ; Pozuelos, Francisco J ; Raup, Zachary ; Reed, Phillip ; Relles, Howard M ; Ricker, George R ; Savel, Arjun B ; Schwarz, Richard P ; Seager, Sara ; Sefako, Ramotholo ; Srdoc, Gregor ; Stockdale, Chris ; Sullivan, Hannah ; Timmermans, Mathilde ; Winn, Joshua N</creator><creatorcontrib>Schulte, Jack ; Rodriguez, Joseph E ; Bieryla, Allyson ; Quinn, Samuel N ; Collins, Karen A ; Yee, Samuel W ; Nine, Andrew C ; Soares-Furtado, Melinda ; Latham, David W ; Eastman, Jason D ; Barkaoui, Khalid ; Ciardi, David R ; Dragomir, Diana ; Everett, Mark E ; Giacalone, Steven ; Mireles, Ismael ; Murgas, Felipe ; Narita, Norio ; Shporer, Avi ; Strakhov, Ivan A ; Striegel, Stephanie ; Vaňko, Martin ; Vowell, Noah ; Wang, Gavin ; Ziegler, Carl ; Bellaver, Michael ; Benni, Paul ; Bergeron, Serge ; Boffin, Henri M. J ; Briceño, César ; Clark, Catherine A ; Collins, Kevin I ; de Leon, Jerome P ; Dressing, Courtney D ; Evans, Phil ; Esparza-Borges, Emma ; Fedewa, Jeremy ; Fukui, Akihiko ; Gan, Tianjun ; Gerasimov, Ivan S ; Hartman, Joel D ; Gill, Holden ; Gillon, Michaël ; Horne, Keith ; Horta, Ferran Grau ; Howell, Steve B ; Isogai, Keisuke ; Jehin, Emmanuël ; Jenkins, Jon M ; Karjalainen, Raine ; Kielkopf, John F ; Lester, Kathryn V ; Littlefield, Colin ; Lund, Michael B ; Mann, Andrew W ; McCormack, Mason ; Michaels, Edward J ; Painter, Shane ; Palle, Enric ; Parviainen, Hannu ; Peterson, David-Michael ; Pozuelos, Francisco J ; Raup, Zachary ; Reed, Phillip ; Relles, Howard M ; Ricker, George R ; Savel, Arjun B ; Schwarz, Richard P ; Seager, Sara ; Sefako, Ramotholo ; Srdoc, Gregor ; Stockdale, Chris ; Sullivan, Hannah ; Timmermans, Mathilde ; Winn, Joshua N</creatorcontrib><description><![CDATA[Hot Jupiters were many of the first exoplanets discovered in the 1990s, but
in the decades since their discovery, the mysteries surrounding their origins
remain. Here, we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b,
TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and
TOI-5301 b) discovered by NASA's TESS mission and confirmed using ground-based
imaging and spectroscopy. These discoveries are the first in a series of papers
named the Migration and Evolution of giant ExoPlanets (MEEP) survey and are
part of an ongoing effort to build a complete sample of hot Jupiters orbiting
FGK stars, with a limiting Gaia $G$-band magnitude of 12.5. This effort aims to
use homogeneous detection and analysis techniques to generate a set of
precisely measured stellar and planetary properties that is ripe for
statistical analysis. The nine planets presented in this work occupy a range of
masses (0.55 Jupiter masses (M$_{\rm{J}}$) $<$ M$_{\rm{P}}$ $<$ 3.88
M$_{\rm{J}}$) and sizes (0.967 Jupiter radii (R$_{\rm{J}}$) $<$ R$_{\rm{P}}$
$<$ 1.438 R$_{\rm{J}}$) and orbit stars that range in temperature from 5360 K
$<$ Teff $<$ 6860 K with Gaia $G$-band magnitudes ranging from 11.1 to 12.7.
Two of the planets in our sample have detectable orbital eccentricity: TOI-3919
b ($e = 0.259^{+0.033}_{-0.036}$) and TOI-5301 b ($e = 0.33^{+0.11}_{-0.10}$).
These eccentric planets join a growing sample of eccentric hot Jupiters that
are consistent with high-eccentricity tidal migration, one of the three most
prominent theories explaining hot Jupiter formation and evolution.]]></description><identifier>DOI: 10.48550/arxiv.2401.05923</identifier><language>eng</language><subject>Physics - Earth and Planetary Astrophysics</subject><creationdate>2024-01</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2401.05923$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2401.05923$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Schulte, Jack</creatorcontrib><creatorcontrib>Rodriguez, Joseph E</creatorcontrib><creatorcontrib>Bieryla, Allyson</creatorcontrib><creatorcontrib>Quinn, Samuel N</creatorcontrib><creatorcontrib>Collins, Karen A</creatorcontrib><creatorcontrib>Yee, Samuel W</creatorcontrib><creatorcontrib>Nine, Andrew C</creatorcontrib><creatorcontrib>Soares-Furtado, Melinda</creatorcontrib><creatorcontrib>Latham, David W</creatorcontrib><creatorcontrib>Eastman, Jason D</creatorcontrib><creatorcontrib>Barkaoui, Khalid</creatorcontrib><creatorcontrib>Ciardi, David R</creatorcontrib><creatorcontrib>Dragomir, Diana</creatorcontrib><creatorcontrib>Everett, Mark E</creatorcontrib><creatorcontrib>Giacalone, Steven</creatorcontrib><creatorcontrib>Mireles, Ismael</creatorcontrib><creatorcontrib>Murgas, Felipe</creatorcontrib><creatorcontrib>Narita, Norio</creatorcontrib><creatorcontrib>Shporer, Avi</creatorcontrib><creatorcontrib>Strakhov, Ivan A</creatorcontrib><creatorcontrib>Striegel, Stephanie</creatorcontrib><creatorcontrib>Vaňko, Martin</creatorcontrib><creatorcontrib>Vowell, Noah</creatorcontrib><creatorcontrib>Wang, Gavin</creatorcontrib><creatorcontrib>Ziegler, Carl</creatorcontrib><creatorcontrib>Bellaver, Michael</creatorcontrib><creatorcontrib>Benni, Paul</creatorcontrib><creatorcontrib>Bergeron, Serge</creatorcontrib><creatorcontrib>Boffin, Henri M. J</creatorcontrib><creatorcontrib>Briceño, César</creatorcontrib><creatorcontrib>Clark, Catherine A</creatorcontrib><creatorcontrib>Collins, Kevin I</creatorcontrib><creatorcontrib>de Leon, Jerome P</creatorcontrib><creatorcontrib>Dressing, Courtney D</creatorcontrib><creatorcontrib>Evans, Phil</creatorcontrib><creatorcontrib>Esparza-Borges, Emma</creatorcontrib><creatorcontrib>Fedewa, Jeremy</creatorcontrib><creatorcontrib>Fukui, Akihiko</creatorcontrib><creatorcontrib>Gan, Tianjun</creatorcontrib><creatorcontrib>Gerasimov, Ivan S</creatorcontrib><creatorcontrib>Hartman, Joel D</creatorcontrib><creatorcontrib>Gill, Holden</creatorcontrib><creatorcontrib>Gillon, Michaël</creatorcontrib><creatorcontrib>Horne, Keith</creatorcontrib><creatorcontrib>Horta, Ferran Grau</creatorcontrib><creatorcontrib>Howell, Steve B</creatorcontrib><creatorcontrib>Isogai, Keisuke</creatorcontrib><creatorcontrib>Jehin, Emmanuël</creatorcontrib><creatorcontrib>Jenkins, Jon M</creatorcontrib><creatorcontrib>Karjalainen, Raine</creatorcontrib><creatorcontrib>Kielkopf, John F</creatorcontrib><creatorcontrib>Lester, Kathryn V</creatorcontrib><creatorcontrib>Littlefield, Colin</creatorcontrib><creatorcontrib>Lund, Michael B</creatorcontrib><creatorcontrib>Mann, Andrew W</creatorcontrib><creatorcontrib>McCormack, Mason</creatorcontrib><creatorcontrib>Michaels, Edward J</creatorcontrib><creatorcontrib>Painter, Shane</creatorcontrib><creatorcontrib>Palle, Enric</creatorcontrib><creatorcontrib>Parviainen, Hannu</creatorcontrib><creatorcontrib>Peterson, David-Michael</creatorcontrib><creatorcontrib>Pozuelos, Francisco J</creatorcontrib><creatorcontrib>Raup, Zachary</creatorcontrib><creatorcontrib>Reed, Phillip</creatorcontrib><creatorcontrib>Relles, Howard M</creatorcontrib><creatorcontrib>Ricker, George R</creatorcontrib><creatorcontrib>Savel, Arjun B</creatorcontrib><creatorcontrib>Schwarz, Richard P</creatorcontrib><creatorcontrib>Seager, Sara</creatorcontrib><creatorcontrib>Sefako, Ramotholo</creatorcontrib><creatorcontrib>Srdoc, Gregor</creatorcontrib><creatorcontrib>Stockdale, Chris</creatorcontrib><creatorcontrib>Sullivan, Hannah</creatorcontrib><creatorcontrib>Timmermans, Mathilde</creatorcontrib><creatorcontrib>Winn, Joshua N</creatorcontrib><title>Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission</title><description><![CDATA[Hot Jupiters were many of the first exoplanets discovered in the 1990s, but
in the decades since their discovery, the mysteries surrounding their origins
remain. Here, we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b,
TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and
TOI-5301 b) discovered by NASA's TESS mission and confirmed using ground-based
imaging and spectroscopy. These discoveries are the first in a series of papers
named the Migration and Evolution of giant ExoPlanets (MEEP) survey and are
part of an ongoing effort to build a complete sample of hot Jupiters orbiting
FGK stars, with a limiting Gaia $G$-band magnitude of 12.5. This effort aims to
use homogeneous detection and analysis techniques to generate a set of
precisely measured stellar and planetary properties that is ripe for
statistical analysis. The nine planets presented in this work occupy a range of
masses (0.55 Jupiter masses (M$_{\rm{J}}$) $<$ M$_{\rm{P}}$ $<$ 3.88
M$_{\rm{J}}$) and sizes (0.967 Jupiter radii (R$_{\rm{J}}$) $<$ R$_{\rm{P}}$
$<$ 1.438 R$_{\rm{J}}$) and orbit stars that range in temperature from 5360 K
$<$ Teff $<$ 6860 K with Gaia $G$-band magnitudes ranging from 11.1 to 12.7.
Two of the planets in our sample have detectable orbital eccentricity: TOI-3919
b ($e = 0.259^{+0.033}_{-0.036}$) and TOI-5301 b ($e = 0.33^{+0.11}_{-0.10}$).
These eccentric planets join a growing sample of eccentric hot Jupiters that
are consistent with high-eccentricity tidal migration, one of the three most
prominent theories explaining hot Jupiter formation and evolution.]]></description><subject>Physics - Earth and Planetary Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj0FPgzAYhnvxYKY_wJPfUQ9goVCKN0OqmxlzybiTj1FmE2iX0s3t32-ipzfv5cnzEPIQ0TARaUpf0J30MYwTGoU0zWN2S4ZS7xx6bQ2gaUEebX-Ynu1gp9F4kCe77tEoP8JTKeX6GRavsNJGwUr99GcorOm0G1QLc-vh87DXXrkROmcH8N8KKrnZQKnH8Uq9Izcd9qO6_98Zqd5lVcyD5dfHonhbBsgzFqiGxUJklEVZm_H4aspZI3JFm1hkGGEskOYoFFUtZ12T0DzdcmwYxTThbbRlM_L4h516673TA7pz_dtdT93sAhByUZ8</recordid><startdate>20240111</startdate><enddate>20240111</enddate><creator>Schulte, Jack</creator><creator>Rodriguez, Joseph E</creator><creator>Bieryla, Allyson</creator><creator>Quinn, Samuel N</creator><creator>Collins, Karen A</creator><creator>Yee, Samuel W</creator><creator>Nine, Andrew C</creator><creator>Soares-Furtado, Melinda</creator><creator>Latham, David W</creator><creator>Eastman, Jason D</creator><creator>Barkaoui, Khalid</creator><creator>Ciardi, David R</creator><creator>Dragomir, Diana</creator><creator>Everett, Mark E</creator><creator>Giacalone, Steven</creator><creator>Mireles, Ismael</creator><creator>Murgas, Felipe</creator><creator>Narita, Norio</creator><creator>Shporer, Avi</creator><creator>Strakhov, Ivan A</creator><creator>Striegel, Stephanie</creator><creator>Vaňko, Martin</creator><creator>Vowell, Noah</creator><creator>Wang, Gavin</creator><creator>Ziegler, Carl</creator><creator>Bellaver, Michael</creator><creator>Benni, Paul</creator><creator>Bergeron, Serge</creator><creator>Boffin, Henri M. J</creator><creator>Briceño, César</creator><creator>Clark, Catherine A</creator><creator>Collins, Kevin I</creator><creator>de Leon, Jerome P</creator><creator>Dressing, Courtney D</creator><creator>Evans, Phil</creator><creator>Esparza-Borges, Emma</creator><creator>Fedewa, Jeremy</creator><creator>Fukui, Akihiko</creator><creator>Gan, Tianjun</creator><creator>Gerasimov, Ivan S</creator><creator>Hartman, Joel D</creator><creator>Gill, Holden</creator><creator>Gillon, Michaël</creator><creator>Horne, Keith</creator><creator>Horta, Ferran Grau</creator><creator>Howell, Steve B</creator><creator>Isogai, Keisuke</creator><creator>Jehin, Emmanuël</creator><creator>Jenkins, Jon M</creator><creator>Karjalainen, Raine</creator><creator>Kielkopf, John F</creator><creator>Lester, Kathryn V</creator><creator>Littlefield, Colin</creator><creator>Lund, Michael B</creator><creator>Mann, Andrew W</creator><creator>McCormack, Mason</creator><creator>Michaels, Edward J</creator><creator>Painter, Shane</creator><creator>Palle, Enric</creator><creator>Parviainen, Hannu</creator><creator>Peterson, David-Michael</creator><creator>Pozuelos, Francisco J</creator><creator>Raup, Zachary</creator><creator>Reed, Phillip</creator><creator>Relles, Howard M</creator><creator>Ricker, George R</creator><creator>Savel, Arjun B</creator><creator>Schwarz, Richard P</creator><creator>Seager, Sara</creator><creator>Sefako, Ramotholo</creator><creator>Srdoc, Gregor</creator><creator>Stockdale, Chris</creator><creator>Sullivan, Hannah</creator><creator>Timmermans, Mathilde</creator><creator>Winn, Joshua N</creator><scope>GOX</scope></search><sort><creationdate>20240111</creationdate><title>Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission</title><author>Schulte, Jack ; Rodriguez, Joseph E ; Bieryla, Allyson ; Quinn, Samuel N ; Collins, Karen A ; Yee, Samuel W ; Nine, Andrew C ; Soares-Furtado, Melinda ; Latham, David W ; Eastman, Jason D ; Barkaoui, Khalid ; Ciardi, David R ; Dragomir, Diana ; Everett, Mark E ; Giacalone, Steven ; Mireles, Ismael ; Murgas, Felipe ; Narita, Norio ; Shporer, Avi ; Strakhov, Ivan A ; Striegel, Stephanie ; Vaňko, Martin ; Vowell, Noah ; Wang, Gavin ; Ziegler, Carl ; Bellaver, Michael ; Benni, Paul ; Bergeron, Serge ; Boffin, Henri M. J ; Briceño, César ; Clark, Catherine A ; Collins, Kevin I ; de Leon, Jerome P ; Dressing, Courtney D ; Evans, Phil ; Esparza-Borges, Emma ; Fedewa, Jeremy ; Fukui, Akihiko ; Gan, Tianjun ; Gerasimov, Ivan S ; Hartman, Joel D ; Gill, Holden ; Gillon, Michaël ; Horne, Keith ; Horta, Ferran Grau ; Howell, Steve B ; Isogai, Keisuke ; Jehin, Emmanuël ; Jenkins, Jon M ; Karjalainen, Raine ; Kielkopf, John F ; Lester, Kathryn V ; Littlefield, Colin ; Lund, Michael B ; Mann, Andrew W ; McCormack, Mason ; Michaels, Edward J ; Painter, Shane ; Palle, Enric ; Parviainen, Hannu ; Peterson, David-Michael ; Pozuelos, Francisco J ; Raup, Zachary ; Reed, Phillip ; Relles, Howard M ; Ricker, George R ; Savel, Arjun B ; Schwarz, Richard P ; Seager, Sara ; Sefako, Ramotholo ; Srdoc, Gregor ; Stockdale, Chris ; Sullivan, Hannah ; Timmermans, Mathilde ; Winn, Joshua N</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a673-eb328870317d76205963b89e0b287a1a28a09a8e0ed63fb4095c6ab30a546d1c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Physics - Earth and Planetary Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Schulte, Jack</creatorcontrib><creatorcontrib>Rodriguez, Joseph E</creatorcontrib><creatorcontrib>Bieryla, Allyson</creatorcontrib><creatorcontrib>Quinn, Samuel N</creatorcontrib><creatorcontrib>Collins, Karen A</creatorcontrib><creatorcontrib>Yee, Samuel W</creatorcontrib><creatorcontrib>Nine, Andrew C</creatorcontrib><creatorcontrib>Soares-Furtado, Melinda</creatorcontrib><creatorcontrib>Latham, David W</creatorcontrib><creatorcontrib>Eastman, Jason D</creatorcontrib><creatorcontrib>Barkaoui, Khalid</creatorcontrib><creatorcontrib>Ciardi, David R</creatorcontrib><creatorcontrib>Dragomir, Diana</creatorcontrib><creatorcontrib>Everett, Mark E</creatorcontrib><creatorcontrib>Giacalone, Steven</creatorcontrib><creatorcontrib>Mireles, Ismael</creatorcontrib><creatorcontrib>Murgas, Felipe</creatorcontrib><creatorcontrib>Narita, Norio</creatorcontrib><creatorcontrib>Shporer, Avi</creatorcontrib><creatorcontrib>Strakhov, Ivan A</creatorcontrib><creatorcontrib>Striegel, Stephanie</creatorcontrib><creatorcontrib>Vaňko, Martin</creatorcontrib><creatorcontrib>Vowell, Noah</creatorcontrib><creatorcontrib>Wang, Gavin</creatorcontrib><creatorcontrib>Ziegler, Carl</creatorcontrib><creatorcontrib>Bellaver, Michael</creatorcontrib><creatorcontrib>Benni, Paul</creatorcontrib><creatorcontrib>Bergeron, Serge</creatorcontrib><creatorcontrib>Boffin, Henri M. J</creatorcontrib><creatorcontrib>Briceño, César</creatorcontrib><creatorcontrib>Clark, Catherine A</creatorcontrib><creatorcontrib>Collins, Kevin I</creatorcontrib><creatorcontrib>de Leon, Jerome P</creatorcontrib><creatorcontrib>Dressing, Courtney D</creatorcontrib><creatorcontrib>Evans, Phil</creatorcontrib><creatorcontrib>Esparza-Borges, Emma</creatorcontrib><creatorcontrib>Fedewa, Jeremy</creatorcontrib><creatorcontrib>Fukui, Akihiko</creatorcontrib><creatorcontrib>Gan, Tianjun</creatorcontrib><creatorcontrib>Gerasimov, Ivan S</creatorcontrib><creatorcontrib>Hartman, Joel D</creatorcontrib><creatorcontrib>Gill, Holden</creatorcontrib><creatorcontrib>Gillon, Michaël</creatorcontrib><creatorcontrib>Horne, Keith</creatorcontrib><creatorcontrib>Horta, Ferran Grau</creatorcontrib><creatorcontrib>Howell, Steve B</creatorcontrib><creatorcontrib>Isogai, Keisuke</creatorcontrib><creatorcontrib>Jehin, Emmanuël</creatorcontrib><creatorcontrib>Jenkins, Jon M</creatorcontrib><creatorcontrib>Karjalainen, Raine</creatorcontrib><creatorcontrib>Kielkopf, John F</creatorcontrib><creatorcontrib>Lester, Kathryn V</creatorcontrib><creatorcontrib>Littlefield, Colin</creatorcontrib><creatorcontrib>Lund, Michael B</creatorcontrib><creatorcontrib>Mann, Andrew W</creatorcontrib><creatorcontrib>McCormack, Mason</creatorcontrib><creatorcontrib>Michaels, Edward J</creatorcontrib><creatorcontrib>Painter, Shane</creatorcontrib><creatorcontrib>Palle, Enric</creatorcontrib><creatorcontrib>Parviainen, Hannu</creatorcontrib><creatorcontrib>Peterson, David-Michael</creatorcontrib><creatorcontrib>Pozuelos, Francisco J</creatorcontrib><creatorcontrib>Raup, Zachary</creatorcontrib><creatorcontrib>Reed, Phillip</creatorcontrib><creatorcontrib>Relles, Howard M</creatorcontrib><creatorcontrib>Ricker, George R</creatorcontrib><creatorcontrib>Savel, Arjun B</creatorcontrib><creatorcontrib>Schwarz, Richard P</creatorcontrib><creatorcontrib>Seager, Sara</creatorcontrib><creatorcontrib>Sefako, Ramotholo</creatorcontrib><creatorcontrib>Srdoc, Gregor</creatorcontrib><creatorcontrib>Stockdale, Chris</creatorcontrib><creatorcontrib>Sullivan, Hannah</creatorcontrib><creatorcontrib>Timmermans, Mathilde</creatorcontrib><creatorcontrib>Winn, Joshua N</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Schulte, Jack</au><au>Rodriguez, Joseph E</au><au>Bieryla, Allyson</au><au>Quinn, Samuel N</au><au>Collins, Karen A</au><au>Yee, Samuel W</au><au>Nine, Andrew C</au><au>Soares-Furtado, Melinda</au><au>Latham, David W</au><au>Eastman, Jason D</au><au>Barkaoui, Khalid</au><au>Ciardi, David R</au><au>Dragomir, Diana</au><au>Everett, Mark E</au><au>Giacalone, Steven</au><au>Mireles, Ismael</au><au>Murgas, Felipe</au><au>Narita, Norio</au><au>Shporer, Avi</au><au>Strakhov, Ivan A</au><au>Striegel, Stephanie</au><au>Vaňko, Martin</au><au>Vowell, Noah</au><au>Wang, Gavin</au><au>Ziegler, Carl</au><au>Bellaver, Michael</au><au>Benni, Paul</au><au>Bergeron, Serge</au><au>Boffin, Henri M. J</au><au>Briceño, César</au><au>Clark, Catherine A</au><au>Collins, Kevin I</au><au>de Leon, Jerome P</au><au>Dressing, Courtney D</au><au>Evans, Phil</au><au>Esparza-Borges, Emma</au><au>Fedewa, Jeremy</au><au>Fukui, Akihiko</au><au>Gan, Tianjun</au><au>Gerasimov, Ivan S</au><au>Hartman, Joel D</au><au>Gill, Holden</au><au>Gillon, Michaël</au><au>Horne, Keith</au><au>Horta, Ferran Grau</au><au>Howell, Steve B</au><au>Isogai, Keisuke</au><au>Jehin, Emmanuël</au><au>Jenkins, Jon M</au><au>Karjalainen, Raine</au><au>Kielkopf, John F</au><au>Lester, Kathryn V</au><au>Littlefield, Colin</au><au>Lund, Michael B</au><au>Mann, Andrew W</au><au>McCormack, Mason</au><au>Michaels, Edward J</au><au>Painter, Shane</au><au>Palle, Enric</au><au>Parviainen, Hannu</au><au>Peterson, David-Michael</au><au>Pozuelos, Francisco J</au><au>Raup, Zachary</au><au>Reed, Phillip</au><au>Relles, Howard M</au><au>Ricker, George R</au><au>Savel, Arjun B</au><au>Schwarz, Richard P</au><au>Seager, Sara</au><au>Sefako, Ramotholo</au><au>Srdoc, Gregor</au><au>Stockdale, Chris</au><au>Sullivan, Hannah</au><au>Timmermans, Mathilde</au><au>Winn, Joshua N</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission</atitle><date>2024-01-11</date><risdate>2024</risdate><abstract><![CDATA[Hot Jupiters were many of the first exoplanets discovered in the 1990s, but
in the decades since their discovery, the mysteries surrounding their origins
remain. Here, we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b,
TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and
TOI-5301 b) discovered by NASA's TESS mission and confirmed using ground-based
imaging and spectroscopy. These discoveries are the first in a series of papers
named the Migration and Evolution of giant ExoPlanets (MEEP) survey and are
part of an ongoing effort to build a complete sample of hot Jupiters orbiting
FGK stars, with a limiting Gaia $G$-band magnitude of 12.5. This effort aims to
use homogeneous detection and analysis techniques to generate a set of
precisely measured stellar and planetary properties that is ripe for
statistical analysis. The nine planets presented in this work occupy a range of
masses (0.55 Jupiter masses (M$_{\rm{J}}$) $<$ M$_{\rm{P}}$ $<$ 3.88
M$_{\rm{J}}$) and sizes (0.967 Jupiter radii (R$_{\rm{J}}$) $<$ R$_{\rm{P}}$
$<$ 1.438 R$_{\rm{J}}$) and orbit stars that range in temperature from 5360 K
$<$ Teff $<$ 6860 K with Gaia $G$-band magnitudes ranging from 11.1 to 12.7.
Two of the planets in our sample have detectable orbital eccentricity: TOI-3919
b ($e = 0.259^{+0.033}_{-0.036}$) and TOI-5301 b ($e = 0.33^{+0.11}_{-0.10}$).
These eccentric planets join a growing sample of eccentric hot Jupiters that
are consistent with high-eccentricity tidal migration, one of the three most
prominent theories explaining hot Jupiter formation and evolution.]]></abstract><doi>10.48550/arxiv.2401.05923</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.2401.05923 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_2401_05923 |
| source | arXiv.org |
| subjects | Physics - Earth and Planetary Astrophysics |
| title | Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission |
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